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Kinematics of stars in the Pleiades open cluster. / Loktin, A.
In: Astronomy Reports, Vol. 50, No. 9, 2006, p. 714-721.

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Harvard

Loktin, A 2006, 'Kinematics of stars in the Pleiades open cluster', Astronomy Reports, vol. 50, no. 9, pp. 714-721. https://doi.org/10.1134/S1063772906090058

APA

Loktin, A. (2006). Kinematics of stars in the Pleiades open cluster. Astronomy Reports, 50(9), 714-721. https://doi.org/10.1134/S1063772906090058

Vancouver

Loktin A. Kinematics of stars in the Pleiades open cluster. Astronomy Reports. 2006;50(9):714-721. doi: 10.1134/S1063772906090058

Author

Loktin, A. / Kinematics of stars in the Pleiades open cluster. In: Astronomy Reports. 2006 ; Vol. 50, No. 9. pp. 714-721.

BibTeX

@article{a6cf444467144880800db5e72d19eeef,
title = "Kinematics of stars in the Pleiades open cluster",
abstract = "A master catalog of stellar proper motions in the field of the Pleiades young open cluster has been created based on data adopted from 12 catalogs. A total of 340 likely cluster members are identified, 80% with linear-velocity components in the plane of the sky estimated to better than 0.7 km/s. The average radial and tangential motions are analyzed. No rotation of the cluster or expansion or compression of the cluster as a whole or of its parts was found. The dispersion of the residual velocities does not depend on the masses of the stars, as is demonstrated by an absence of mass segregation in the spatial distribution of the stars in the cluster. Most of the stellar orbits in the cluster are strongly elongated.",
author = "A. Loktin",
year = "2006",
doi = "10.1134/S1063772906090058",
language = "English",
volume = "50",
pages = "714--721",
journal = "Astronomy Reports",
issn = "1063-7729",
publisher = "Pleiades Publishing",
number = "9",

}

RIS

TY - JOUR

T1 - Kinematics of stars in the Pleiades open cluster

AU - Loktin, A.

PY - 2006

Y1 - 2006

N2 - A master catalog of stellar proper motions in the field of the Pleiades young open cluster has been created based on data adopted from 12 catalogs. A total of 340 likely cluster members are identified, 80% with linear-velocity components in the plane of the sky estimated to better than 0.7 km/s. The average radial and tangential motions are analyzed. No rotation of the cluster or expansion or compression of the cluster as a whole or of its parts was found. The dispersion of the residual velocities does not depend on the masses of the stars, as is demonstrated by an absence of mass segregation in the spatial distribution of the stars in the cluster. Most of the stellar orbits in the cluster are strongly elongated.

AB - A master catalog of stellar proper motions in the field of the Pleiades young open cluster has been created based on data adopted from 12 catalogs. A total of 340 likely cluster members are identified, 80% with linear-velocity components in the plane of the sky estimated to better than 0.7 km/s. The average radial and tangential motions are analyzed. No rotation of the cluster or expansion or compression of the cluster as a whole or of its parts was found. The dispersion of the residual velocities does not depend on the masses of the stars, as is demonstrated by an absence of mass segregation in the spatial distribution of the stars in the cluster. Most of the stellar orbits in the cluster are strongly elongated.

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UR - http://www.scopus.com/inward/record.url?partnerID=8YFLogxK&scp=33748765859

U2 - 10.1134/S1063772906090058

DO - 10.1134/S1063772906090058

M3 - Article

VL - 50

SP - 714

EP - 721

JO - Astronomy Reports

JF - Astronomy Reports

SN - 1063-7729

IS - 9

ER -

ID: 42252158